Neutrino flavor conversion in supernova 1987A

Details Neutrino flavor conversion in supernova 1987A Neutrino flavor conversion in supernova 1987A

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrvd..38.3605m&link_type=abstract

Physical Review D (Particles and Fields), Volume 38, Issue 12, 15 December 1988, pp.3605-3609

Physics

25

Supernovae

Scientific paper

By using detailed models of the progenitor we show that the non-adiabatic solution of the solar-neutrino problem by the Mikheyev-Smirnov-Wolfenstein mechanism is compatible with the possible observation of neutronization νe from SN 1987A in its wide range of the mixing parameters at Δm2>~10-6 eV2. We also argue that, under the assumption of hierarchy of neutrino masses, our consistency solution favors the νe-heaviest-flavor-neutrino mixing as the cause of the solar-neutrino deficit.

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